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- W2916069811 abstract "In the EeV range, neutrinos are expected to be produced by ultra-high energy cosmic rays interactions with the Cosmic Microwave Background during propagation in the Universe. We report on the search for ultra-high energy neutrinos in data collected with the Surface Detector of the Pierre Auger Observatory. The searches are most efficient in the zenith angle range from 60 degrees to 95 degrees with tau neutrinos skimming in the Earth playing a dominant role. The present non-detection of UHE neutrinos in the Pierre Auger Observatory excludes the most optimistic scenarios of neutrino production in terms of UHE cosmic rays chemical composition and cosmological evolution of the acceleration sites. We also report on the searches for neutrinos in coincidence with the recent Gravitational Wave events detected by LIGO/Virgo." @default.
- W2916069811 created "2019-03-02" @default.
- W2916069811 creator A5068965189 @default.
- W2916069811 date "2019-02-22" @default.
- W2916069811 modified "2023-09-25" @default.
- W2916069811 title "Ultra-high energy neutrinos searches with the Pierre Auger Observatory" @default.
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- W2916069811 doi "https://doi.org/10.21468/scipostphysproc.1.047" @default.
- W2916069811 hasPublicationYear "2019" @default.
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